Centroid motion test results for Kepler-62f in the Q1–Q17 DR25 data set are shown in Fig. REF . The transit signature is clearly visible in the detrended and phase folded flux displayed in the top panel, but there is little discernible centroid shift in either right ascension or declination. The magnitude of the peak centroid shift was determined to be \(0.294 \pm 0.338\)  mas. The total centroid motion detection statistic was reported to be 2.57 for which the significance is \(p = 0.28\)  (not statistically significant). The magnitude of the source offset from the KIC position of the target was estimated to be 1.08 arcsec (1.50\(\sigma \) ). The fitted transit depth for this confirmed HZ super-Earth [1]} was \(470 \pm 31\)  ppm.
